eShel III system (motorized focuser)

24 052,80 € incl. VAT - 20 044,00 € excl. VAT

The eShel III spectrograph is a professional-grade, multi-wavelength fibre-optic instrument.
When it is not possible to choose between resolution and spectral range, as is the case, for example, in the study of exoplanets, an Echelle spectroscope is required, as it provides numerous high-resolution orders (R = 10,000).
The eShel spectroscope covers a range of approximately 370 to 910 nm (orders 25 to 60).

The complete eShel system comprises the spectroscope itself, as well as the guide cap (F/6), the calibration module (with ThAr lamp), the high-voltage power supply and the optical fibres (20 m long).

Complete your spectroscope with the products below :

Recommended acquisition cameras

Recommended cameras: technical specifications

Description Shelyak ref. Included
Acc. type
Cooled
Comment
Camera Atik 460EX Mono SE0124 Camera Science yes The standard CCD camera for the eShel II
Caméra ASI2600MM-Pro EL0271 Camera Science yes New generation CMOS camera

All about the product:

Description

A fiber-fed spectroscope

The eShel III spectroscope enables work across a wide spectral range (370 to 910 nm) at high resolution (R = 10,000). This is made possible by the use of multiple orders (in this case, between 25 and 60); an Echelle spectrum can be read ‘like a book’: the end of one order is found at the start of the next.

The decision was taken to adopt a fibre-optic solution in order to improve the accuracy of radial velocity measurements (the instrument is separate from the telescope, ideally housed in a temperature-controlled room, and is therefore not subject to any flexure) and to enhance user comfort.

We have developed this instrument based on our experience with the Musicos and Narval professional spectroscopes.

Echelle spectroscopy

This technique enables high spectral resolution to be achieved as it use the higher diffraction orders of a diffraction grating. The resulting spectrum passes through a cross disperser, which “slices” the spectrum into successive orders, occupying the entire surface of the camera’s sensor. In this way, the entire spectral range in the visible spectrum is obtained over some twenty orders (in the case of the eShel).

eShel III optical path

Schematic diagram of an Echelle spectrograph (© François Cochard)

The eShel III spectroscope

This is the main module that generates the Echelle spectrum. It covers the spectral range from approximately 370 to 910 nm with a resolution of R=10,000 (using an ASI 2600 MM Pro camera, not included). It has an FC/PC connector for attaching 50 µm object fiber.

Example using the solar spectrum

Sunlight spectrum

Orders #22 through #61 are uniformly focused.

Spectrum of Chi Oph Be star

This allows us to process orders #25 through #60 and extend the usable spectral range from approximately 370 to 910 nm. The motorised version of this lens comes with a PrimaLuce Lab focuser, which allows for remote focusing (ideal for remote operation or when the spectrograph is not located next to the control PC).
There is also a manual version fitted with a helical focuser.

Applications

  • High-resolution spectrum of variable stars
  • Time series of the pulsating star (RR Lyr)
  • Radial velocities calculation
  • High-resolution solar spectrum
  • Be stars survey
  • Planetary nebulae
  • Spectral classification of stars
  • Classification of asteroids
  • Lunar geology
  • Planets composition
  • Abundance measurement
  • Novae
  • RR Lyrae
  • Herbig Ae/Be
  • T Tauri
  • Wolf Rayet

 

Specifications

Petzval lens with a focal length of 122 mm @ f/2.2

  • PrimaLuce Lab motorised focuser
  • Requires the use of a SONY IMX571 sensor (we recommend the ASI 2600 MM Pro), which is not supplied with the eShel III
  • Resolution Power R = 10 000
  • Spectral range covered: approximately 370 to 910 nm
  • FC connector for 50µm object fiber
  • Weight of the eShel III spectrograph on its own (excluding the camera): 4.4 kg
  • 50µm fibre injection FIGU (FC connector) at F/6 and autoguiding (excluding camera)
  • 50µm fibre (20m long) with FC connectors at both ends
  • 200µm calibration fibre (20m long) with FC connectors at both ends
  • Calibration unit with a thorium/argon hollow-cathode lamp and a flat halogen lamp
  • Cables and power supplies compliant with the European standard (220V). To be adapted for other formats
  • Optional cameras (guiding and science camera)

Composition

  • the Eshel III, with its Petval optical system featuring a 122mm focal length and its PrimaLuce Lab motorised focuser
  • 1 interface board for an ASI 2600 MM Pro camera
  • the tools required to adjust the spectrograph
  • The calibration module, with its high-voltage power supply and thorium/argon lamp
  • The 50µm fibre-optic injection adapterat f/6 with autoguiding
  • The various power cables, and the 20-metre-long connection cable between the microphone and the calibration module
  • 50µm-diameter optical fibre (20m long)
  • 200µm Calibration optical fibre (length 20m)
  • The M42 T variable adapter ring

Software

Articles related to this product:

Demetra tutorial

Demetra tutorial

You'll find all our Demetra video tutorials on this web page. Demetra is a free software package for processing spectra from the ALPY 600, LISA and eShel spectrographs from the Shelyak Instruments range. Playlist of Demetra tutorials Tutorial #1 Introduction to...

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